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- W2166669096 abstract "We present the results of a systematic search for pulsating components in Algol-type eclipsing binary systems. A total number of 14 eclipsing binaries with A–F spectral type primary components were observed for 22 nights. We confirmed small-amplitude oscillating features of a recently detected pulsator TW Dra, which has a pulsating period of 0.053 day and a semi-amplitude of about 5 mmag in B-passband. We discovered new pulsating components in two eclipsing binaries of RX Hya and AB Per. The primary component of RX Hya is pulsating with a dominant period of 0.052 day and a semi-amplitude of about 7 mmag. AB Per has also a pulsating component with a period of 0.196 day and a semi-amplitude of about 10 mmag in B-passband. We suggest that these two new pulsators are members of the newly introduced group of mass-accreting pulsating stars in semi-detached Algol-type eclipsing binary systems." @default.
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- W2166669096 date "2003-06-16" @default.
- W2166669096 modified "2023-09-30" @default.
- W2166669096 title "Search for A–F Spectral type pulsating components in Algol-type eclipsing binary systems" @default.
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- W2166669096 doi "https://doi.org/10.1051/0004-6361:20030630" @default.
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